Exciting New Images from The LROC Team.

Frozen impact melt flows on the ejecta blanket of the young impact crater Giordano Bruno (22 km diameter). The image is about 600 m across and the flows are about 50-100 m wide (NASA/GSFC/Arizona State University).

A northeast-trending wrinkle ridge cuts across the plains of Mare Imbrium. The overall ridge is about 4.5 km wide. The contact between the ridge (right) and the surrounding mare basalt plains (left) runs diagonally up the image (NASA/GSFC/Arizona State University).

Dark materials excavated by later small impacts show up clearly on the bright ejecta of a small lunar crater (800 meters in diameter) to the west. Image width is 640 meters [NASA/GSFC/Arizona State University].

As the Apollo 11 Lunar Module (LM) neared the surface, Neil Armstrong could see the landing area was right on the rough bouldery ejecta of West crater. He had to change the flight plan and fly the LM westward to find a safe landing spot. Image 742 meters wide, north is up [NASA/GSFC/Arizona State University].